The Boltzmann equation and Cosmic Microwave Background
Observations on the anisotropies of the Cosmic Microwave Background (CMB) have become a fundamental tool in Cosmology. We present a brief description of the mformalism necessary to understand the evolution of the anisotropies, and how their power spectrum gives us information about the evolution and...
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2023 |
| País: | Perú |
| Institución: | Universidad Nacional Mayor de San Marcos |
| Repositorio: | Revistas - Universidad Nacional Mayor de San Marcos |
| Idioma: | inglés |
| OAI Identifier: | oai:revistasinvestigacion.unmsm.edu.pe:article/23631 |
| Acceso en línea: | https://revistasinvestigacion.unmsm.edu.pe/index.php/fisica/article/view/23631 |
| Access Level: | acceso abierto |
| Palabra clave: | Cosmology cosmic microwave background Boltzmann equation Cosmología radiacion del fondo cósmico ecuación de Boltzmann |
| Sumario: | Observations on the anisotropies of the Cosmic Microwave Background (CMB) have become a fundamental tool in Cosmology. We present a brief description of the mformalism necessary to understand the evolution of the anisotropies, and how their power spectrum gives us information about the evolution and composition of the universe. |
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